To construct a two-dimensional model of the density and temperature in the
torus, the 9 different particle species yield 9 equations of the form
(10) which, completed with the equation of charge neutrality, permit us
to calculate the normalized density profiles along the magnetic field
. The normalized temperature profiles
are then obtained using the 9
corresponding equations of the form (11) or (12).
Details of the calculation are given in the appendix.
Since the model has two dimensions, we may distinguish between input
parameters
concerning the radial dependency (namely the equatorial density
and temperatures
,
at a given Jovicentric distance) and
those concerning the latitudinal dependency of the model (namely
and
at an altitude
from the centrifugal equator)
which both depend on the magnetic field geometry and on the bi-kappa
distribution parameters
and
.